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Table 5
Orbital and Gaia DR1 details on the 256 planets analysed with GASTON.
| RV data | Gaia DR1 data | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Name | P | m sin i | K | e | ω | Tp | M⋆ | ap | π | a⋆ sin i | Transit | Drift | εDR1 | Npts | NFoV | Gaia | Duplicate |
| (days) | (MJ) | (m s−1) | (°) | − 2 450 000 | (M⊙) | (au) | (mas) | (mas) | flag | flag | (mas) | dataset | source | ||||
| 30 Ari B b | 335.1 ± 2.5 | 9.88 ± 0.98 | 272 ± 24 | 0.289 ± 0.092 | 307 ± 18 | 4538 ± 20 | 1.160 ± 0.040 | 0.992 ± 0.012 | 21.42 ± 0.60 | 0.173 ± 0.019 | n | n | 1.8 | 71 | 10 | 1 | n |
| HAT-P-21 b | 4.1244810 ± 0.0000070 | 4.07 ± 0.17 | 548 ± 14 | 0.228 ± 0.016 | 309.0 ± 3.0 | 4995.014 ± 0.046 | 0.947 ± 0.042 | 0.04943 ± 0.00073 | 3.73 ± 0.51 | 0.00076 ± 0.00011 | n | n | 0.92 | 84 | 10 | 1 | n |
| HD 114762 b | 83.9151 ± 0.0030 | 11.64 ± 0.78 | 612.5 ± 3.5 | 0.3354 ± 0.0048 | 201.3 ± 1.0 | −110.89 ± 0.19 | 0.895 ± 0.089 | 0.361 ± 0.012 | 25.88 ± 0.46 | 0.116 ± 0.015 | n | n | 1.1 | 130 | 23 | 1 | n |
| HD 132563 B b | 1544 ± 34 | 1.49 ± 0.14 | 26.7 ± 2.2 | 0.220 ± 0.090 | 158 ± 35 | 2593 ± 148 | 1.010 ± 0.010 | 2.623 ± 0.039 | 9.30 ± 0.33 | 0.0344 ± 0.0034 | n | n | 0.85 | 130 | 19 | 1 | y |
| HD 141937 b | 653.2 ± 1.2 | 9.48 ± 0.41 | 234.5 ± 6.4 | 0.410 ± 0.010 | 187.72 ± 0.80 | 1847.4 ± 2.0 | 1.048 ± 0.037 | 1.497 ± 0.018 | 30.62 ± 0.35 | 0.396 ± 0.023 | n | n | 0.93 | 236 | 32 | 1 | y |
| HD 148427 b | 331.5 ± 3.0 | 1.144 ± 0.092 | 27.7 ± 2.0 | 0.160 ± 0.080 | 277 ± 68 | 3991 ± 15 | 1.360 ± 0.060 | 1.039 ± 0.017 | 14.17 ± 0.42 | 0.0118 ± 0.0012 | n | n | 1.1 | 131 | 17 | 1 | n |
| HD 154857 b | 408.60 ± 0.50 | 2.248 ± 0.092 | 48.3 ± 1.0 | 0.460 ± 0.020 | 57.0 ± 4.0 | 3572.5 ± 2.4 | 1.718 ± 0.026 | 1.2907 ± 0.0066 | 15.56 ± 0.39 | 0.0251 ± 0.0013 | n | n | 0.93 | 122 | 19 | 1 | n |
| HD 154857 c | 3452 ± 105 | 2.58 ± 0.15 | 24.2 ± 1.1 | 0.060 ± 0.050 | 352 ± 37 | 5219 ± 375 | 1.718 ± 0.026 | 5.35 ± 0.11 | 15.56 ± 0.39 | 0.1194 ± 0.0081 | n | n | 0.93 | 122 | 19 | 1 | n |
| HD 164595 b | 40.00 ± 0.24 | 0.0508 ± 0.0070 | 3.05 ± 0.41 | 0.088 ± 0.093 | 145 ± 135 | 6280 ± 12 | 0.990 ± 0.030 | 0.2281 ± 0.0025 | 35.11 ± 0.38 | 0.000392 ± 0.000056 | n | n | 0.93 | 62 | 8 | 1 | y |
| HD 16760 b | 465.1 ± 2.3 | 13.29 ± 0.61 | 408.0 ± 7.0 | 0.067 ± 0.010 | 232 ± 10 | 4723 ± 12 | 0.780 ± 0.050 | 1.081 ± 0.023 | 14 | 0.25 | n | n | 3.0 | 62 | 10 | 2 | n |
| HD 177830 b | 410.1 ± 2.2 | 1.320 ± 0.085 | 32.64 ± 0.98 | 0.096 ± 0.048 | 189 | 254 ± 49 | 1.17 ± 0.10 | 1.138 ± 0.033 | 15.94 ± 0.37 | 0.0195 ± 0.0022 | n | n | 0.87 | 89 | 19 | 1 | n |
| HD 185269 b | 6.8379 ± 0.0010 | 0.954 ± 0.069 | 90.7 ± 4.4 | 0.296 ± 0.040 | 172 ± 11 | 3154.089 ± 0.040 | 1.28 ± 0.10 | 0.0766 ± 0.0020 | 19.10 ± 0.41 | 0.00104 ± 0.00012 | n | n | 0.97 | 74 | 16 | 1 | n |
| HD 190228 b | 1136.1 ± 9.9 | 5.94 ± 0.30 | 91.4 ± 3.0 | 0.531 ± 0.028 | 101.2 ± 2.1 | 3522 ± 12 | 1.821 ± 0.046 | 2.602 ± 0.027 | 15.77 ± 0.34 | 0.1278 ± 0.0079 | n | n | 0.86 | 116 | 16 | 1 | y |
| HD 197037 b | 1036 ± 13 | 0.807 ± 0.060 | 15.5 ± 1.0 | 0.220 ± 0.070 | 298 ± 26 | 1353 ± 86 | 1.1 | 2.1 | 30.01 ± 0.32 | 0.043 | n | n | 0.99 | 107 | 17 | 1 | n |
| HD 4203 b | 431.88 ± 0.85 | 2.08 ± 0.12 | 60.3 ± 2.2 | 0.519 ± 0.027 | 329.1 ± 3.0 | 1918.9 ± 2.7 | 1.130 ± 0.064 | 1.165 ± 0.022 | 12.67 ± 0.44 | 0.0259 ± 0.0023 | n | n | 0.85 | 60 | 11 | 1 | n |
| HD 5388 b | 777.0 ± 4.0 | 1.97 ± 0.10 | 41.7 ± 1.6 | 0.400 ± 0.020 | 324.0 ± 4.0 | 4570.0 ± 9.0 | 1.2 | 1.8 | 18.86 ± 0.32 | 0.052 | n | n | 1.4 | 327 | 48 | 1 | y |
| HD 6718 b | 2496 ± 176 | 1.56 ± 0.12 | 24.1 ± 1.5 | 0.100 ± 0.075 | 286 ± 50 | 4357 ± 251 | 0.96 | 3.6 | 19.74 ± 0.41 | 0.11 | n | n | 1.1 | 199 | 29 | 1 | y |
| HD 7449 b | 1275 ± 13 | 1.31 ± 0.52 | 42 ± 15 | 0.820 ± 0.060 | 339.0 ± 6.0 | 5298 ± 26 | 1.1 | 2.3 | 27.14 ± 0.41 | 0.076 | n | n | 0.94 | 61 | 12 | 1 | y |
| HD 95127 b | 482.0 ± 5.0 | 5.04 ± 0.82 | 116 ± 12 | 0.11 ± 0.10 | 40 ± 38 | 3200 ± 50 | 1.20 ± 0.22 | 1.278 ± 0.079 | 1.31 ± 0.58 | 0.0067 ± 0.0034 | n | n | 1.2 | 41 | 8 | 1 | n |
| HD 96127 b | 647 ± 17 | 4.01 ± 0.85 | 105 ± 11 | 0.30 ± 0.10 | 162 ± 18 | 3969 ± 31 | 0.91 ± 0.25 | 1.42 ± 0.13 | 1.87 ± 0.83 | 0.0112 ± 0.0064 | n | n | 1.1 | 109 | 16 | 1 | n |
| HIP 65891 b | 1084 ± 23 | 6.00 ± 0.41 | 64.9 ± 2.4 | 0.130 ± 0.050 | 356 ± 16 | 6015 ± 49 | 2.50 ± 0.21 | 2.804 ± 0.088 | 6.53 ± 0.37 | 0.0420 ± 0.0053 | n | n | 1.1 | 237 | 35 | 1 | n |
| K2-110 b | 13.86375 ± 0.00026 | 0.053 ± 0.011 | 5.5 ± 1.1 | 0.079 ± 0.070 | 90 ± 122 | 6863 | 0.738 ± 0.018 | 0.10207 ± 0.00083 | 8.6 | 0.000060 | n | n | 1.3 | 54 | 9 | 2 | y |
| K2-34 b | 2.9956290 ± 0.0000060 | 1.683 ± 0.061 | 207.0 ± 3.0 | 0.000 ± 0.027 | 90 | 7144.347030 ± 0.000080 | 1.226 ± 0.052 | 0.04353 ± 0.00062 | 3.28 ± 0.68 | 0.000187 ± 0.000040 | n | n | 1.00 | 117 | 16 | 1 | y |
| WASP-11 b | 3.7224650 ± 0.0000070 | 0.540 ± 0.052 | 82.1 ± 7.4 | 0 | 90 | 4473.05588 ± 0.00020 | 0.800 ± 0.025 | 0.04364 ± 0.00045 | 7.49 ± 0.58 | 0.000211 ± 0.000027 | n | n | 1.1 | 60 | 10 | 1 | n |
| WASP-131 b | 5.3220230 ± 0.0000050 | 0.272 ± 0.018 | 30.5 ± 1.7 | 0 | 90 | 6919.82360 ± 0.00040 | 1.060 ± 0.060 | 0.0608 ± 0.0011 | 4.55 ± 0.56 | 0.000068 ± 0.000010 | n | n | 0.95 | 53 | 7 | 1 | n |
| WASP-156 b | 3.8361690 ± 0.0000030 | 0.1305 ± 0.0087 | 19.0 ± 1.0 | 0.0000 ± 0.0035 | 90 | 4677.7070 ± 0.0020 | 0.842 ± 0.052 | 0.04529 ± 0.00093 | 8.2 | 0.000055 | n | n | 1.5 | 38 | 7 | 2 | n |
| WASP-157 b | 3.9516205 ± 0.0000040 | 0.559 ± 0.049 | 61.6 ± 3.8 | 0.000 ± 0.055 | 90 | 7257.803194 ± 0.000088 | 1.26 ± 0.12 | 0.0528 ± 0.0017 | 3.76 ± 0.66 | 0.000084 ± 0.000019 | n | n | 0.87 | 69 | 9 | 1 | n |
| WASP-17 b | 3.7354330 ± 0.0000076 | 0.508 ± 0.030 | 59.2 ± 2.9 | 0 | 90 | 4559.18096 ± 0.00023 | 1.190 ± 0.030 | 0.04993 ± 0.00042 | 2.57 ± 0.31 | 0.0000523 ± 0.0000072 | n | n | 0.85 | 202 | 25 | 1 | n |
| WASP-43 b | 0.8134750 ± 0.0000010 | 1.76 ± 0.10 | 550.3 ± 6.7 | 0 | 90 | 5528.86774 ± 0.00014 | 0.580 ± 0.050 | 0.01422 ± 0.00041 | 11 | 0.00047 | n | n | 2.0 | 63 | 7 | 2 | n |
Notes. We only show here the 29 planets belonging to the “detection” sample, i.e. for which the astrometric excess noise surpasses the detection threshold (see Table 6). The full table, including the 227 planets from the “non-detection” sample, i.e. for which the astrometric excess noise is smaller than the threshold, is available at the CDS. Where uncertainties are missing we assume 10%errors on the corresponding parameter. The parallax with uncertainties are all taken from the DR1, while those without uncertainties are taken from SIMBAD. Orbit references can be found in the full-version of Table 2 at the CDS.
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